The density variance-mach number relation in supersonic, isothermal turbulence

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dc.contributor.authorPrice, Daniel J.
dc.contributor.authorFederrath, Christoph
dc.contributor.authorBrunt, C M
dc.date.accessioned2018-11-29T22:56:39Z
dc.date.available2018-11-29T22:56:39Z
dc.date.issued2011
dc.date.updated2018-11-29T08:13:31Z
dc.format.mimetypeapplication/pdfen_AU
dc.identifier.issn2041-8205
dc.identifier.urihttp://hdl.handle.net/1885/153589
dc.publisherInstitute of Physics Publishing Ltd.
dc.sourceAstrophysical Journal Letters
dc.subjectKeywords: Hydrodynamics; ISM: structure; Magnetohydrodynamics (MHD); Shock waves; Stars: formation; Turbulence
dc.titleThe density variance-mach number relation in supersonic, isothermal turbulence
dc.typeJournal article
dcterms.accessRightsOpen Accessen_AU
local.bibliographicCitation.issue1
local.bibliographicCitation.lastpage5
local.bibliographicCitation.startpage1
local.contributor.affiliationPrice, Daniel J., Monash University
local.contributor.affiliationFederrath, Christoph, College of Science, ANU
local.contributor.affiliationBrunt, C M, University of Exeter
local.contributor.authoremailu5575624@anu.edu.au
local.contributor.authoruidFederrath, Christoph, u5575624
local.description.notesImported from ARIES
local.identifier.absfor020104 - Galactic Astronomy
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.absfor020199 - Astronomical and Space Sciences not elsewhere classified
local.identifier.absseo970102 - Expanding Knowledge in the Physical Sciences
local.identifier.ariespublicationU3488905xPUB15287
local.identifier.citationvolume727
local.identifier.doi10.1088/2041-8205/727/1/L21
local.identifier.scopusID2-s2.0-79960254999
local.identifier.thomsonID000285993800021
local.identifier.uidSubmittedByU3488905
local.type.statusPublished Version

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